Zobrazeno 1 - 10
of 1 803
pro vyhledávání: '"Cai, Zheng"'
Autor:
Sillassen, Nikolaj B., Jin, Shuowen, Magdis, Georgios E., Daddi, Emanuele, Wang, Tao, Lu, Shiying, Sun, Hanwen, Arumugam, Vinod, Liu, Daizhong, Brinch, Malte, D'Eugenio, Chiara, Gobat, Raphael, Gómez-Guijarro, Carlos, Rich, Michael, Schinnerer, Eva, Strazzullo, Veronica, Tan, Qinghua, Valentino, Francesco, Wang, Yijun, Xiao, Mengyuan, Zhou, Luwenjia, Blánquez-Sesé, David, Cai, Zheng, Chen, Yanmei, Ciesla, Laure, Dai, Yu, Delvecchio, Ivan, Elbaz, David, Finoguenov, Alexis, Gao, Fangyou, Gu, Qiusheng, Hale, Catherine, Hao, Qiaoyang, Huang, Jiasheng, Jarvis, Matt, Kalita, Boris, Ke, Xu, Bail, Aurelien Le, Magnelli, Benjamin, Shi, Yong, Vaccari, Mattia, Whittam, Imogen, Yang, Tiancheng, Zhang, Zhiyu
The NOEMA formIng Cluster survEy (NICE) is a large program targeting 69 massive galaxy group candidates at $z>2$ in six deep fields. We report spectroscopic confirmation of eight groups at $1.65\leq z\leq3.61$ in COSMOS. Homogeneously selected as sig
Externí odkaz:
http://arxiv.org/abs/2407.02973
Being the most prominent HI line, Ly$\alpha$ permeates the cosmic web in emission. Despite its potential as a cosmological probe, its detection on large scales remains elusive. We present a new methodology to perform Ly$\alpha$ intensity mapping with
Externí odkaz:
http://arxiv.org/abs/2406.18775
Identifying and predicting the factors that contribute to the success of interdisciplinary research is crucial for advancing scientific discovery. However, there is a lack of methods to quantify the integration of new ideas and technological advancem
Externí odkaz:
http://arxiv.org/abs/2406.01391
Autor:
Li, Mingyu, Zhang, Haibin, Cai, Zheng, Liang, Yongming, Kashikawa, Nobunari, Ma, Ke, Fan, Xiaohui, Prochaska, J. Xavier, Emonts, Bjorn H. C., Wang, Xin, Wu, Yunjing, Zhang, Shiwu, Li, Qiong, Johnson, Sean D., Yue, Minghao, Battaia, Fabrizio Arrigoni, Cantalupo, Sebastiano, Hennawi, Joseph F., Kikuta, Satoshi, Ning, Yuanhang, Ouchi, Masami, Shimakawa, Rhythm, Wang, Ben, Wang, Weichen, Zheng, Zheng, Zheng, Zhen-Ya
Circumgalactic Lyman-alpha (Ly$\alpha$) nebulae are gaseous halos around galaxies exhibiting luminous extended Ly$\alpha$ emission. This work investigates Ly$\alpha$ nebulae from deep imaging of $\sim12~\mathrm{deg}^2$ sky, targeted by the MAMMOTH-Su
Externí odkaz:
http://arxiv.org/abs/2405.13113
Autor:
Jiang, Linhua, Fu, Shuqi, Wang, Feige, Bosman, Sarah E. I., Cai, Zheng, Jun, Hyunsung D., Pan, Zhiwei, Sun, Fengwu, Yang, Jinyi, Zhang, Huanian
We present constraints on the spacetime variation of the fine-structure constant $\alpha$ at redshifts $3
Externí odkaz:
http://arxiv.org/abs/2405.08977
Autor:
Pudoka, Maria, Wang, Feige, Fan, Xiaohui, Yang, Jinyi, Champagne, Jaclyn, Jones, Victoria, Bian, Fuyan, Cai, Zheng, Jiang, Linhua, Liu, Dezi, Wu, Xue-Bing
We study the environment of the z=6.33 ultraluminous quasar SDSS J010013.02+280225.8 (J0100) to understand its association with large-scale structure. Theoretical models propose high-redshift quasars as markers of galaxy overdensities residing in the
Externí odkaz:
http://arxiv.org/abs/2405.03781
Autor:
Liang, Yongming, Ouchi, Masami, Sun, Dongsheng, Kashikawa, Nobunari, Cai, Zheng, Cantalupo, Sebastiano, Nagamine, Kentaro, Yajima, Hidenobu, Kirihara, Takanobu, Zhang, Haibin, Li, Mingyu, Shimakawa, Rhythm, Fan, Xiaohui, Ito, Kei, Tanaka, Masayuki, Harikane, Yuichi, Prochaska, J. Xavier, Travascio, Andrea, Wang, Weichen, Elvis, Martin, Fabbiano, Giuseppina, Arita, Junya, Onoue, Masafusa, Silverman, John D., Shi, Dongdong, An, FangXia, Izumi, Takuma, Shimasaku, Kazuhiro, Uchiyama, Hisakazu, Zhu, Chenghao
We report the identification of a quasar overdensity in the BOSSJ0210 field, dubbed Cosmic Himalayas, consisting of 11 quasars at $z=2.16-2.20$, the densest overdensity of quasars ($17\sigma$) in the $\sim$10,000 deg$^2$ of the Sloan Digital Sky Surv
Externí odkaz:
http://arxiv.org/abs/2404.15963
Autor:
Fudamoto, Yoshinobu, Sun, Fengwu, Diego, Jose M., Dai, Liang, Oguri, Masamune, Zitrin, Adi, Zackrisson, Erik, Jauzac, Mathilde, Lagattuta, David J., Egami, Eiichi, Iani, Edoardo, Windhorst, Rogier A., Abe, Katsuya T., Bauer, Franz Erik, Bian, Fuyan, Bhatawdekar, Rachana, Broadhurst, Thomas J., Cai, Zheng, Chen, Chian-Chou, Chen, Wenlei, Cohen, Seth H., Conselice, Christopher J., Espada, Daniel, Foo, Nicholas, Frye, Brenda L., Fujimoto, Seiji, Furtak, Lukas J., Golubchik, Miriam, Hsiao, Tiger Yu-Yang, Jolly, Jean-Baptiste, Kawai, Hiroki, Kelly, Patrick L., Koekemoer, Anton M., Kohno, Kotaro, Kokorev, Vasily, Li, Mingyu, Li, Zihao, Lin, Xiaojing, Magdis, Georgios E., Meena, Ashish K., Nabizadeh, Armin, Richard, Johan, Steinhardt, Charles L., Wu, Yunjing, Zhu, Yongda, Zou, Siwei
Strong gravitational magnification by massive galaxy clusters enable us to detect faint background sources, resolve their detailed internal structures, and in the most extreme cases identify and study individual stars in distant galaxies. Highly magn
Externí odkaz:
http://arxiv.org/abs/2404.08045
Autor:
Cai, Zheng, Cao, Maosong, Chen, Haojiong, Chen, Kai, Chen, Keyu, Chen, Xin, Chen, Xun, Chen, Zehui, Chen, Zhi, Chu, Pei, Dong, Xiaoyi, Duan, Haodong, Fan, Qi, Fei, Zhaoye, Gao, Yang, Ge, Jiaye, Gu, Chenya, Gu, Yuzhe, Gui, Tao, Guo, Aijia, Guo, Qipeng, He, Conghui, Hu, Yingfan, Huang, Ting, Jiang, Tao, Jiao, Penglong, Jin, Zhenjiang, Lei, Zhikai, Li, Jiaxing, Li, Jingwen, Li, Linyang, Li, Shuaibin, Li, Wei, Li, Yining, Liu, Hongwei, Liu, Jiangning, Hong, Jiawei, Liu, Kaiwen, Liu, Kuikun, Liu, Xiaoran, Lv, Chengqi, Lv, Haijun, Lv, Kai, Ma, Li, Ma, Runyuan, Ma, Zerun, Ning, Wenchang, Ouyang, Linke, Qiu, Jiantao, Qu, Yuan, Shang, Fukai, Shao, Yunfan, Song, Demin, Song, Zifan, Sui, Zhihao, Sun, Peng, Sun, Yu, Tang, Huanze, Wang, Bin, Wang, Guoteng, Wang, Jiaqi, Wang, Jiayu, Wang, Rui, Wang, Yudong, Wang, Ziyi, Wei, Xingjian, Weng, Qizhen, Wu, Fan, Xiong, Yingtong, Xu, Chao, Xu, Ruiliang, Yan, Hang, Yan, Yirong, Yang, Xiaogui, Ye, Haochen, Ying, Huaiyuan, Yu, Jia, Yu, Jing, Zang, Yuhang, Zhang, Chuyu, Zhang, Li, Zhang, Pan, Zhang, Peng, Zhang, Ruijie, Zhang, Shuo, Zhang, Songyang, Zhang, Wenjian, Zhang, Wenwei, Zhang, Xingcheng, Zhang, Xinyue, Zhao, Hui, Zhao, Qian, Zhao, Xiaomeng, Zhou, Fengzhe, Zhou, Zaida, Zhuo, Jingming, Zou, Yicheng, Qiu, Xipeng, Qiao, Yu, Lin, Dahua
The evolution of Large Language Models (LLMs) like ChatGPT and GPT-4 has sparked discussions on the advent of Artificial General Intelligence (AGI). However, replicating such advancements in open-source models has been challenging. This paper introdu
Externí odkaz:
http://arxiv.org/abs/2403.17297
Autor:
Wang, Tao, Sun, Hanwen, Zhou, Luwenjia, Xu, Ke, Cheng, Cheng, Li, Zhaozhou, Chen, Yangyao, Mo, H. J., Dekel, Avishai, Zheng, Xianzhong, Cai, Zheng, Yang, Tiacheng, Dai, Y. -S., Elbaz, David, Huang, J. -S.
One of the main challenges in galaxy formation that has emerged recently is the early assembly of massive galaxies. The observed number density and the maximum stellar mass ($M_{\star}$) of massive galaxies in the early Universe appear to be higher t
Externí odkaz:
http://arxiv.org/abs/2403.02399